1. Chapter 3 – Energy Balance and Temperature

2. The Fate of Solar Radiation We owe it all to the sun… 3 things can happen to solar (and all) radiation: 1) Absorption 2) Scattering and Reflection 3) Transmission

3. Absorption Absorption – the full energy transfer from radiation to a substance Getting hotter…

4. Absorption Absorption – the full energy transfer from radiation to a substance Atmospheric absorption varies by substance: Getting hotter…

5. Absorption Absorption – the full energy transfer from radiation to a substance Atmospheric absorption varies by substance: UV – absorbed by O 3 (stratosphere) Getting hotter…

6. Absorption Absorption – the full energy transfer from radiation to a substance Atmospheric absorption varies by substance: UV – absorbed by O 3 (stratosphere) Visible – hardly absorbed (lucky for us) Getting hotter…

7. Absorption Absorption – the full energy transfer from radiation to a substance Atmospheric absorption varies by substance: UV – absorbed by O 3 (stratosphere) Visible – hardly absorbed (lucky for us) Infrared – partially absorbed by water vapor, CO 2 (less cooling in high humidity..) Getting hotter…

8. Absorption – The Atmospheric Window The atmospheric window is a band (8-12 μm) of very little absorption Earth’s surface emissionAtmospheric absorption

9. Absorption – The Atmospheric Window Liquid water (i.e. clouds), however, are good absorbers of all longwave radiation

10. Absorption – The Atmospheric Window Liquid water (i.e. clouds), however, are good absorbers of all longwave radiation Are cloudy or clear nights warmer???

11. Scattering and Reflection Scattering – the deflection of radiation by a substance

12. Scattering and Reflection Scattering – the deflection of radiation by a substance Diffuse scattering – radiation deflected in many directions, becomes diffuse radiation

13. Scattering and Reflection Scattering – the deflection of radiation by a substance Diffuse scattering – radiation deflected in many directions, becomes diffuse radiation Reflection – a type of scattering, radiation is deflected back with equal intensity (mirror)

14. Scattering and Reflection Scattering – the deflection of radiation by a substance Diffuse scattering – radiation deflected in many directions, becomes diffuse radiation Reflection – a type of scattering, radiation is deflected back with equal intensity (mirror) Albedo – the fraction of light reflected (earth’s albedo is ~0.3)

15. Scattering and Reflection Scattering affects many things: Shaded areas still receive solar radiation (better buy more sunscreen!)

16. Scattering and Reflection Scattering affects many things: Shaded areas still receive solar radiation (better buy more sunscreen!) The sky is blue and sunsets are red (Rayleigh scattering)

17. Scattering and Reflection Scattering affects many things: Shaded areas still receive solar radiation (better buy more sunscreen!) The sky is blue and sunsets are red (Rayleigh scattering) Hazy or polluted days make the sky white or gray (Mie scattering)

18. Scattering and Reflection Scattering affects many things: Shaded areas still receive solar radiation (better buy more sunscreen!) The sky is blue and sunsets are red (Rayleigh scattering) Hazy or polluted days make the sky white or gray (Mie scattering) Clouds are white (nonselective scattering)

19. Rayleigh Scattering -Occurs when substance is small compared to wavelength of radiation (such as atmospheric gases)

20. Rayleigh Scattering -Occurs when substance is small compared to wavelength of radiation (such as atmospheric gases) -Scatters smaller wavelengths (blue) more than longer wavelengths (red)

21. Rayleigh Scattering -Occurs when substance is small compared to wavelength of radiation (such as atmospheric gases) -Scatters smaller wavelengths (blue) more than longer wavelengths (red) -Makes the sky appear blue, sunsets red

22. Rayleigh Scattering

24. Mie Scattering -Occurs when substance is of comparable size to wavelength of radiation (such as aerosols)

25. Mie Scattering -Occurs when substance is of comparable size to wavelength of radiation (such as aerosols) -Unlike Rayleigh scattering, scatters all wavelengths more efficiently

26. Mie Scattering -Occurs when substance is of comparable size to wavelength of radiation (such as aerosols) -Unlike Rayleigh scattering, scatters all wavelengths more efficiently -Makes hazy and polluted skies look white or gray, enhances sunsets

27. Mie Scattering

28. Nonselective Scattering -Scattering by relatively large particles such as cloud droplets -Scatters all wavelengths comparably -Makes clouds white or gray

29. Transmission Transmission – radiation passes through a substance without being absorbed or scattered

30. The Energy Balance of Earth Earth is generally neither warming or cooling (global climate change aside) – it is in steady-state, or equilibrium (just like a skydiver at terminal velocity…)

31. The Energy Balance of Earth Earth is generally neither warming or cooling (global climate change aside) – it is in steady-state, or equilibrium (just like a skydiver at terminal velocity…) This means the gain from solar radiation must be balanced by the loss from terrestrial radiation

32. The Energy Balance of Earth The story begins with a net gain of solar radiation…

33. The Energy Balance of Earth The story ends with a loss of longwave radiation from earth and the atmosphere

34. The Energy Balance of Earth But the story isn’t really over….

35. The Energy Balance of Earth But the story isn’t really over…. In this situation, the atmosphere and surface will cool and heat indefinitely…

36. The Energy Balance of Earth But the story isn’t really over…. In this situation, the atmosphere and surface will cool and heat indefinitely… - Why don’t they?

37. The Energy Balance of Earth Conduction and convection!!! 1) Conduction causes heat transfer to air in contact with ground

38. The Energy Balance of Earth Conduction and convection!!! 1) Conduction causes heat transfer to air in contact with ground 2) Convection causes this air near the surface to rise like a helium balloon, mixing heat throughout the atmosphere Sensible heat flux

39. The Energy Balance of Earth Conduction and convection!!! 2 types of convection Free convectionForced convection

40. The Energy Balance of Earth One last mechanism of surface/atmosphere heat exchange: - Latent Heat

41. The Energy Balance of Earth One last mechanism of surface/atmosphere heat exchange: - Latent Heat Latent heat is the energy used to change the phase of a substance, and it is transferred in the atmosphere through convection

42. The Energy Balance of Earth Now the story finally ends, at equilibrium… RadiationConduction and Convection

43. The Energy Balance of Earth Let’s get specific – latitudinal variations also exist in the radiation budget

44. The Energy Balance of Earth Let’s get specific – latitudinal variations also exist in the radiation budget But these are opposed by advection of heat through wind and ocean currents

45. The Greenhouse Effect The atmosphere is kind of like a greenhouse, and kind of not

46. The Greenhouse Effect The atmosphere is kind of like a greenhouse, and kind of not Earth stays warm by atmospheric absorption/re-emission

47. The Greenhouse Effect The atmosphere is kind of like a greenhouse, and kind of not Earth stays warm by atmospheric absorption/re-emission Without greenhouse gases, earth’s equilibrium temperature would be much cooler (0 o F instead of 59 o F)

48. The Greenhouse Effect Altering greenhouse gas (i.e. CO 2 ) concentrations in the atmosphere will alter earth’s equilibrium temperature

49. The Greenhouse Effect Altering greenhouse gas (i.e. CO 2 ) concentrations in the atmosphere will alter earth’s equilibrium temperature

50. Global Climate Change The Intergovernmental Panel on Climate Change (IPCC) stated in 2007 that: 1)Average global temperature is increasing (1.33 o F in the last 100 years)

51. Global Climate Change The Intergovernmental Panel on Climate Change (IPCC) stated in 2007 that: 1)Average global temperature is increasing (1.33 o F in the last 100 years) 2)Temperatures are increasing faster now than they did earlier last century

52. Global Climate Change The Intergovernmental Panel on Climate Change (IPCC) stated in 2007 that: 1)Average global temperature is increasing (1.33 o F in the last 100 years) 2)Temperatures are increasing faster now than they did earlier last century 3)Extreme warm events are increasing, extreme cold events are decreasing

53. Global Climate Change The Intergovernmental Panel on Climate Change (IPCC) stated in 2007 that: 1)Average global temperature is increasing (1.33 o F in the last 100 years) 2)Temperatures are increasing faster now than they did earlier last century 3)Extreme warm events are increasing, extreme cold events are decreasing 4)Global snow cover is decreasing

54. Global Climate Change The Intergovernmental Panel on Climate Change (IPCC) stated in 2007 that: 1)Average global temperature is increasing (1.33 o F in the last 100 years) 2)Temperatures are increasing faster now than they did earlier last century 3)Extreme warm events are increasing, extreme cold events are decreasing 4)Global snow cover is decreasing 5)All of the above is very likely due to anthropogenic greenhouse gas emissions

55. Predicted Global Temperature 2000-2100 Greenhouse gas emissions HIGH MEDIUM LOW

56. Global Climate Change Uncertainties still exist for global warming predictions (effect of aerosols, cloud cover, greenhouse gas emission)

57. Global Climate Change Uncertainties still exist for global warming predictions (effect of aerosols, cloud cover, greenhouse gas emission) Local climate change is a very important aspect of current research

58. Temperature Temperature is a measure of the average kinetic energy of a substance

59. Measuring Temperature Mercury (or other fluid) thermometer – measures temperature by fluid expansion/contraction

60. Measuring Temperature Mercury (or other fluid) thermometer – measures temperature by fluid expansion/contraction Bimetallic strip – measures temperature by different contraction/expansion of metal strips

61. Measuring Temperature Thermistor – measure temperature based on resistance to electrical current (fast response)

62. Measuring Temperature Thermistor – measure temperature based on resistance to electrical current (fast response) Radiosondes – box of weather instruments, including a thermistor, placed on weather balloons to measure atmospheric variables aloft

63. Measuring Temperature Instrument shelters used for surface observations

64. More Tidbits on Temperature… Diurnal range – the range of temperatures over the night/day cycle at a given location

65. More Tidbits on Temperature… Highest temperature ever recorded on earth: 136 o F in Libya Lowest temperature ever recorded on earth: -129 o F in Antarctica

66. More Tidbits on Temperature… Highest temperature ever recorded on earth: 136 o F in Libya Lowest temperature ever recorded on earth: -129 o F in Antarctica Highest temperature ever recorded in Texas: 120 o F in Seymour Lowest temperature ever recorded in Texas: -23 o F in Seminole

67. More Tidbits on Temperature… Wind chill index – provides an estimate of the perceived temperature based on actual temperature and wind

68. How Meteorologists Analyze Temperature In the horizontal…

69. How Meteorologists Analyze Temperature In the vertical... Stuve Diagram